Results 81 to 90 of about 995 (187)

Photometric Metallicity and Distance for the Two RR Lyrae in Segue II and Ursa Major II Dwarf Galaxies Based on Multiband Light Curves

open access: yesThe Astronomical Journal
Multiband light curves of two RR Lyrae variables in Segue II and Ursa Major II ultrafaint dwarf galaxies were collected from near simultaneous observations using the Lulin One-meter Telescope in Vgri bands.
Chow-Choong Ngeow, Anupam Bhardwaj
doaj   +1 more source

Predicting light curves of RR Lyrae variables using artificial neural network based interpolation of a grid of pulsation models

open access: green, 2023
Nitesh Kumar   +6 more
openalex   +2 more sources

Stellar Atmospheric Parameters of ∼11,000 RR Lyrae Stars from LAMOST Spectra

open access: yesThe Astrophysical Journal Supplement Series
Accurate determination of the stellar atmospheric parameters of RR Lyrae stars (RRLs) requires short individual exposures of the spectra to mitigate pulsation effects.
Jiangtao Wang   +4 more
doaj   +1 more source

Color–Magnitude Diagram of NGC 205 and Its RR Lyrae Variables

open access: yesThe Astronomical Journal
We present the deepest color–magnitude diagram (CMD) for NGC 205 in the F606W (≈ V ) and F814W (≈ I ) filters. Our archival Hubble Space Telescope/Advanced Camera for Surveys field is centered ∼3 $\mathop{.}\limits^{{\rm{^{\prime} }}}$ 8 northwest of the
Ata Sarajedini
doaj   +1 more source

Classification for 969 Double-mode RR Lyrae Stars from Zwicky Transient Facility

open access: yesThe Astrophysical Journal Supplement Series
RR Lyrae (RRL) variable stars are cornerstone distance indicators. In particular, double-mode RR Lyrae (RRd) stars enable period–luminosity relations (PLRs) that are less sensitive to metallicity, reducing systematic biases in distance measurements ...
Jianxing Zhang   +4 more
doaj   +1 more source

Kinematics of Distant Milky Way Halo RR Lyrae Stars out to 160 kpc

open access: yesThe Astrophysical Journal
We present a kinematical study of the outer halo ( r _GC  ∼ 60–160 kpc) of the Milky Way (MW) based on spectroscopy of 55 RR Lyrae stars using the Echelle Spectrograph and Imager instrument on the Keck II telescope.
Yuting Feng   +6 more
doaj   +1 more source

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